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The Period Change Rate in the RS CVn Binary HD 5303
Published online by Cambridge University Press: 25 April 2016
Abstract
From the observed timings of primary eclipse of HD 5303 we find that its 2.7 day period is increasing at a rate of about one second per year. In this paper we consider the implications of this in terms of mass transfer or mass loss from the system.
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- Galactic and Stellar
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- Copyright © Astronomical Society of Australia 1991
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